Future Instrumentation for Solar and Stellar Research at Radio ...

More documents

Recommendations

Info

6.1 m x 7.0 m Primary Log-periodic Feed 2.4 m Secondary Offset Gregorian Antenna Az-El Drive Shroud (feed can’t see ground or array)
ATA Performance Number of Elements 350 Element Diameter 6.10 m Total Geometric Area 1.02E+04 m^2 Aperture Efficiency 63% Effective Area 6.44E+03 m^2 2.33 K/Jy System Temperature 43 K System Eqiv. Flux Density 18 Jy Ae/Tsys 150 m^2/K Effective Array Diameter 687 m Natural Weighting Frequency 1 10 GHz Primary FoV 3.5 0.4 degree Synthesized Beam Size 108 11 arc sec Number of Beams >4 Continuum Sensitivity BW 0.2 GHz Confusion Flux Limit in 10 sec 0.41 mJy 0.1 mJy at 1.4 GHz Spectral Line Resolution 10 km/s Frequency 1 10 GHz BW 3.E+04 3.E+05 Hz Integration Time 1000 1000 sec RMS brightness 0.70 0.22 K
Page 1 and 2: Future Instrumentation for Solar an
Page 3 and 4: And Beyond … •SKA - Square Kilo
Page 5 and 6: By deploying N antennas over a two
Page 7: The EVLAThe EVLA (Phase 1) Point so
Page 10 and 11: Configurations Nested rings with di
Page 12 and 13: from R. Simon
Page 14 and 15: CARMA Combine the six 10.4 m antenn
Page 16 and 17: The Frequency Agile Solar Radiotele
Page 18 and 19: Strawman FASR Specifications Freque
Page 20 and 21: from J. Lee
Page 22 and 23: FASR Science • Nature & Evolution
Page 24 and 25: Noise storm Bastian et al. (2001)
Page 26 and 27: from Aschwanden & Benz 1997
Page 28 and 29: Status and Plans The NAS/NRC Astron
Page 30 and 31: The ATA The ATA is a project of the
Page 34 and 35: ATA Science • SETI - 100,000 FGK
Page 36 and 37: SM146 Concept (VLA Scientific Memor
Page 38 and 39: SM146 CAPABILITY SM146 SM146 SM146
Page 40 and 41: SKA Finally, it is worth mentioning
Page 42 and 43: Originally conceived as a “red sh

Future Instrumentation for Solar and Stellar Research at Radio ...

Create successful ePaper yourself

Delete template?

Save as template?